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- W2069686088 startingPage "1327" @default.
- W2069686088 abstract "Because of instrumental sensitivity limits and stellar distances, the types of x-ray flares observable on stars have been intrinsically much more energetic than those on the sun. Such enormous events are a useful extrapolation of the solar phenomenon if the underlying assumption is correct that they form a continuous sequence involving similar physical processes as on the sun. The Advanced Satellite for Cosmology and Astrophysics (ASCA), with its greater sensitivity and high-energy response, is now able to test this hypothesis. Direct comparison with solar flares measured by the x-ray-monitoring Geostationary Operational Environmental Satellites (GOES) is possible. The detection of flares on Proxima Centauri that correspond to GOES M-class events on the sun are reported." @default.
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- W2069686088 date "1995-06-02" @default.
- W2069686088 modified "2023-10-16" @default.
- W2069686088 title "Solar-Like M-Class X-ray Flares on Proxima Centauri Observed by the ASCA Satellite" @default.
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- W2069686088 doi "https://doi.org/10.1126/science.268.5215.1327" @default.
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